Pennsylvania State University | 2020 Jun 30
Coronae of supermassive black holes may be the hidden sources of mysterious cosmic neutrinos seen on Earth
The origin of high-energy cosmic neutrinos observed by the IceCube Neutrino Observatory, whose detector is buried deep in the Antarctic ice, is an enigma that has perplexed physicists and astronomers. A new model could help explain the unexpectedly large flux of some of these neutrinos inferred by recent neutrino and gamma-ray data. A paper by Penn State researchers describing the model points to the supermassive black holes found at the cores of active galaxies as the sources of these mysterious neutrinos ...
- NASA Hubble Space Telescope image of Galaxy NGC 1068 with NuSTAR's view of its active black hole shown as an illustration in the zoomed-in inset. A new model suggests that the corona around such supermassive black holes could be the source of high-energy cosmic neutrinos observed by the IceCube Neutrino Observatory. Credit: NASA/ESA/JPL-Caltech
“Neutrinos are subatomic particles so tiny that their mass is nearly zero and they rarely interact with other matter,” said Kohta Murase, assistant professor of physics and of astronomy and astrophysics at Penn State and a member of Center for Multimessenger Astrophysics in the Institute for Gravitation and the Cosmos (IGC), who led the research. “High-energy cosmic neutrinos are created by energetic cosmic-ray accelerators in the universe, which may be extreme astrophysical objects such as black holes and neutron stars. They must be accompanied by gamma rays or electromagnetic waves at lower energies, and even sometimes gravitational waves. So, we expect the levels of these various 'cosmic messengers' that we observe to be related. Interestingly, the IceCube data have indicated an excess emission of neutrinos with energies below 100 teraelectron volt (TeV), compared to the level of corresponding high-energy gamma rays seen by the Fermi Gamma-ray Space Telescope.”
Scientists combine information from all of these cosmic messengers to learn about events in the universe and to reconstruct its evolution in the burgeoning field of “multimessenger astrophysics.” For extreme cosmic events, like massive stellar explosions and jets from supermassive black holes, that create neutrinos, this approach has helped astronomers pinpoint the distant sources and each additional messenger provides additional clues about the details of the phenomena. ...
Hidden Cores of Active Galactic Nuclei as the Origin of Medium-Energy Neutrinos:
Critical Tests with the MeV Gamma-Ray Connection ~ Kohta Murase, Shigeo S. Kimura, Peter Meszaros
- Physical Review Letters 125(01):1101 (03 July 2020) DOI: 10.1103/PhysRevLett.125.011101
arXiv.org > astro-ph > arXiv:1904.04226 > 08 Apr 2019 (v1), 17 Jun 2020 (v2)